Stability of relative equilibria of the full spacecraft dynamics around an asteroid with orbit–attitude coupling

The full dynamics of spacecraft around an asteroid, in which the spacecraft is considered as a rigid body and the gravitational orbit–attitude coupling is taken into account, is of great value and interest in the precise theories of the motion. The spectral stability of the classical relative equilibria of the full spacecraft dynamics around an asteroid is studied with the method of geometric mechanics. The stability conditions are given explicitly based on the characteristic equation of the linear system matrix. It is found that the linearized system decouples into two entirely independent subsystems, which correspond to the motions within and outside the equatorial plane of the asteroid respectively. The system parameters are divided into three groups that describe the traditional stationary orbit stability, the significance of the orbit–attitude coupling and the mass distribution of the spacecraft respectively. The spectral stability of the relative equilibria is investigated numerically with respect to the three groups of system parameters. The relations between the full spacecraft dynamics and the traditional spacecraft dynamics, as well as the effect of the orbit–attitude coupling, are assessed. We find that when the orbit–attitude coupling is strong, the mass distribution of the spacecraft dominates the stability of the relative equilibria; whereas when the orbit–attitude coupling is weak, both the mass distribution and the traditional stationary orbit stability have significant effects on the stability. We also give a criterion to determine whether the orbit–attitude coupling needs to be considered.     

通过非线性解耦实现绕欧拉特征轴旋转的姿态控制系统

利用四元数反馈,就不需要测量三个欧拉角,从而避免结构上和原理上所带来的麻烦,而且可以实现绕欧拉特征轴的大角度机动,绕欧拉特征轴旋转的角行程是最短的。但是,要实现这种机动,姿态控制系统必须是解耦的。     

面阵CCD时序抗弥散方法研究

文章通过讨论n沟道CCD的物理结构以及两种CCD饱和弥散(弥散型饱和状态和表面型饱和状态)的差异,介绍了面阵CCD抗弥散技术,它通过改变垂直转移时序使普通CCD具有抗弥散功能。对采用该技术前后相机抗弥散的实际效果进行了对比,进一步研究了面阵CCD时序抗弥散所必需的表面型饱和高电平偏置电压测定方法、低电平电压偏置测定方法以及时序工作频率标定方法,给出了工程实现的具体途径。总结了时序抗弥散技术的优缺点,列出了该技术的使用范围和限制条件。     

稳态温度场作用下涡轮叶片振动特性的研究

根据一维线性分段插值方法对一维温度场进行分段插值拟合,为有限元方法分析温度场作用下叶片振动问题中温度载荷的施加提供了简化可行的方案,利用有限元方法验证该线性拟合方案的可行性,并采用多种方法对计算结果进行验证分析,对一维稳态温度场的分段插值进行了误差分析,得到稳态温度场作用下叶片振动问题的有限元分析计算方法和温度载荷施加方案。     

中国上市公司收入分配与所有权结构的实证分析

从公司收入分配角度研究不同所有权性质公司的企业利益和员工利益,研究发现不同所有权结构的企业生产效率差异不大,私有企业的企业利益优于国有企业,国有相对控股企业和私有相对控股企业的企业利益与员工利益相对较好,混合制企业的生产效率可能较低,企业利益与员工利益也相对较差.没有发现支持国有控股企业有大量冗员的证据,国企改革取得部分成功.     

放大器中非线性失真的研究

晶体管是非线性器件,在放大信号时会产生非线性失真.针对弱非线性失真,推导了总谐波人(THD)、二阶互调失真(IM2)、三阶互调失真(IM3)和截点(IP3)的表达式,借助于Multisim软件,对晶体管共发放大器、发射极带反馈电阻的失发放大器、差分放大器和发射极间带反馈电阻的差分放大器进行了仿真,并与理论结果作了比较,结果令人满意.     

基于深度学习的航空器异常飞行状态识别

飞行设备快速存取记录仪(Quick Access Recorder,以下简称QAR)保留了原始航班各类重要飞行参数在内的航行信息,使研究分析航空器实时状况和保障飞行质量成为可能。针对QAR数据高维大样本的特点,在如今大数据背景下,除了传统机理建模分析航空器飞行状态外,采用深度学习的方式建立基于数据驱动的航空器飞行状态识别模型,理论与实用意义兼具。通过对真实QAR飞行数据的研究,开发了基于深度稀疏受限玻尔兹曼机的异常飞行状态识别程序。首先利用小波降噪技术对原始飞行数据进行预处理清洗,在一系列典型飞行参数上提取经典时域特征以及小波奇异熵等信息熵特征构成特征集。在此基础上,分别利用经典的线性主元分析技术和深度稀疏玻尔兹曼机对特征集进行有效降维,最后采用四折交叉验证方式,通过高斯过程分类器实现对飞行状态的辨识。实验结果显示,基于深度受限玻尔兹曼机-高斯过程分类的飞行状态识别具有较高分类准确性。     

基于零控脱靶量的大气层外拦截中制导研究

针对大气层外拦截中段采用耗尽关机固体燃料发动机的情况,设计了基于零控脱靶量的鲁棒中制导律。推导了系统状态转移矩阵,通过数值方法求解得到考虑地球扁率J2摄动项的拦截器零控脱靶状态,在此基础上将推力分解到视线方向和垂直视线方向,并根据垂直视线方向需要速度增量大小设计了推力分配比例系数,使得推力方向平稳变化且能快速减小系统的零控脱靶量。仿真表明,所设计的中制导律简单、可靠,便于工程实现,能有效提高拦截精度,并对发动机工作参数具有较强的鲁棒性。     

基于数据的发动机模型匹配方法研究

针对在使用环境条件下发动机部件特性未知的问题,为获得在实际装机条件下的发动机部件特性,采用1种基于参考数据的发动机部件级模型匹配方法,在对测量数据和模型特征分析的基础上,选取适当调整参数,以模型在非设计点的仿真输出与参考数据的匹配精度为目标,通过迭代方法求解部件特性。仿真数据表明:采用基于数据的发动机匹配技术得到的发动机模型,其仿真输出与参考数据的偏差均在允许范围内。利用该方法可以得到在使用条件下的发动机部件特性,为装机状态发动机的仿真预测提供技术支撑。     

An improved numerical method for constructing Halo/Lissajous orbits in a full solar system model

An improved numerical method that can construct Halo/Lissajous orbits in the vicinity of collinear libration points in a full solar system model is investigated. A full solar system gravitational model in the geocentric rotating coordinate system with a clear presentation of the angular velocity relative to the inertial coordinate system is proposed. An alternative way to determine patch points in the multiple shooting method is provided based on a dynamical analysis with Poincare′sections. By employing the new patch points and sequential quadratic programming, Halo orbits for L_1, L_2, and L_3 points as well as Lissajous orbits for L_1 and L_2 points in the EarthMoon system are generated with the proposed full solar system gravitational model to verify the effectiveness of the proposed method.